Search results for "methods: laboratory: molecular"

showing 4 items of 4 documents

Zeeman effect in sulfur monoxide: A tool to probe magnetic fields in star forming regions

2017

[Context] Magnetic fields play a fundamental role in star formation processes and the best method to evaluate their intensity is to measure the Zeeman effect of atomic and molecular lines. However, a direct measurement of the Zeeman spectral pattern from interstellar molecular species is challenging due to the high sensitivity and high spectral resolution required. So far, the Zeeman effect has been detected unambiguously in star forming regions for very few non-masing species, such as OH and CN.

Methods: laboratory: molecularlaboratory: molecular [Methods]Context (language use)ISM: moleculeRadiation01 natural sciences7. Clean energyArticlesymbols.namesakechemistry.chemical_compoundMethods: data analysis0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsPhysics::Atomic PhysicsSpectral resolutiondata analysis [Methods]010303 astronomy & astrophysicsmolecules [ISM]Astrophysics::Galaxy AstrophysicsCondensed Matter::Quantum GasesPhysicsZeeman effectSulfur monoxide010304 chemical physicsSpectrometerStar formationMolecular dataAstronomy and AstrophysicsAstronomy and AstrophysicISM: moleculesMagnetic fieldMagnetic fieldchemistrySpace and Planetary ScienceMagnetic fieldssymbolsAtomic physicsMethods: data analysi
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Chemical Evolution of Interstellar Methanol Ice Analogs upon Ultraviolet Irradiation: The Role of the Substrate

2018

An important issue in the chemistry of interstellar ices is the role of dust materials. In this work, we study the effect of an amorphous water-rich magnesium silicate deposited onto ZnSe windows on the chemical evolution of ultraviolet-irradiated methanol ices. For comparison, we also irradiate similar ices deposited onto bare ZnSe windows. Silicates are produced at relatively low temperatures exploiting a sol-gel technique. The chemical composition of the synthesized material reflects the forsterite stoichiometry. Si-OH groups and magnesium carbonates are incorporated during the process. The results show that the substrate material does affect the chemical evolution of the ice. In particu…

PhysicsAstrochemistryastrochemistryExtinction (astronomy)methods: laboratory: molecularSubstrate (chemistry)Astronomy and AstrophysicsISM: moleculeAstronomy and AstrophysicPhotochemistryultraviolet: ISM01 natural sciencesChemical evolutionchemistry.chemical_compoundchemistrySpace and Planetary Science0103 physical sciencesUltraviolet irradiationdust extinctionMethanol010306 general physics010303 astronomy & astrophysicsThe Astrophysical Journal
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Rare isotopic species of hydrogen sulfide: the rotational spectrum of H236S

2014

The rotational spectrum of the 36 S-bearing isotopologue of hydrogen sulfide (H2S) has been investigated for the first time in the 167 GHz−1.6 THz frequency range, thus providing an accurate and reliable set of spectroscopic parameters. The experimental investigation was backed up by state-of-the-art quantum-chemical calculations, which also allowed us to demonstrate the incorrectness of the previously reported spectroscopic constants. The present results are of suitable accuracy to attempt the astrophysical detection of the isotopic species under consideration. Finally, reliable predictions for the spectroscopic constants of other rare isotopologues of H2S, namely the mono- and bi-deuterat…

Physicsmolecular dataHydrogen sulfideAnalytical chemistrymethods: laboratory: molecularAstronomy and AstrophysicsISM: moleculeAstrophysicschemistry.chemical_compoundchemistrySpace and Planetary ScienceRotational spectrumsubmillimeter: ISMIsotopologuemethods: data analysitechniques: spectroscopicAstronomy & Astrophysics
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Laboratory measurements and astronomical search for the HSO radical

2016

[Context] Despite the fact that many sulfur-bearing molecules, ranging from simple diatomic species up to astronomical complex molecules, have been detected in the interstellar medium, the sulfur chemistry in space is largely unknown and a depletion in the abundance of S-containing species has been observed in the cold, dense interstellar medium. The chemical form of the missing sulfur has yet to be identified.

inorganic chemicalsMethods: laboratory: molecularHydrogenLine: identificationlaboratory: molecular [Methods]chemistry.chemical_elementContext (language use)ISM: moleculeAstrophysics7. Clean energy01 natural sciencesArticleAbundance (ecology)0103 physical sciencesPhysics::Chemical Physicsidentification [Line]Spectral resolutionSubmillimeter: ISM010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsmolecules [ISM]Radio lines: ISMPhysics010304 chemical physicsMolecular dataTriatomic moleculeISM [Submillimeter]AstronomyAstronomy and AstrophysicsAstronomy and AstrophysicSulfurDiatomic moleculeISM: moleculesISM [Radio lines]Interstellar mediumchemistry13. Climate actionSpace and Planetary ScienceAstronomy & Astrophysics
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